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2MASS J17502484-0016151
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Star 2MASS J17502484-0016151

Brown dwarf 2MASS J17502484-0016151 is located 30 light years away from the Sun. It is a single star of spectral class L5.5 , that has typically about 4 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
30 light years

2MASS J17502484-0016151

Spectral class: L5.5

Location +

Ascension iconRight ascension: 17h 50m 24.391s
Declination iconDeclination: -0° 16' 11.837'' (equatorial region)
Parallax iconParallax: 108.581
Distance iconSun distance: 30.038 ly | 9.2 pc
Star position
The position of a star tells us where it appears in the sky, similar to how we use coordinates like latitude and longitude on Earth. In astronomy, the three main coordinates are right ascension, declination and distance. .. icon More about Star position in StellarGuide

Basic characteristic

icon weight
Mass: 5 % M Sun
| 52.4 M Jupiter
 (estimate)
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Star mass
The estimated mass of the star 2MASS J17502484-0016151 is about 5 % of the Sun's mass, or approximately 52.4 Jupiter masses.

The mass of a star is the total amount of matter it contains. It is one of the most important properties of a star, as it determines almost everything about how the star lives, changes, and dies. In astronomy, star mass is usually measured in solar masses (M☉) — where 1 solar mass is equal to the mass of our Sun... icon More about Star mass in StellarGuide
temperature icon
Temperature: 1800 K | 0.31 T Sun
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Star temperature
Surface temperature of 2MASS J17502484-0016151 is 1800 K, which is 31 % of the temperature on the surface of the Sun.

The temperature of a star refers to the temperature at its surface, also called the photosphere. It is measured in kelvins (K), the standard unit for temperature in astronomy. A star’s temperature tells us a lot about its physical properties and where it stands in its evolutionary stage... icon More about Star temperature in StellarGuide

Photometry

Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).
5
10
15
20
25
30
35
K
2.1
H
1.6
J
1.2
Grp
0.8
I
0.8
G
0.6
V
0.5
Gbp
0.5
B
0.4
U
0.3
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2MASS J17502484-0016151 system structure

2MASS J17502484-0016151

More about 2MASS J17502484-0016151

Temperature on its surface is around 1800 K (1527 °C), which is about 31 % of Sun's temperature.
       2MASS J17502484-0016151 can be found in southern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope. 
Other designations of this star
TIC 39591415, WISEA J175024.53-001612.8, Gaia EDR3 4371611781971072768
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External sources
simbad icon
Simbad database (2MASS J17502484-0016151)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia EDR3 4371611781971072768)
Archive from the Gaia mission

Frequently Asked Questions

How far is the 2MASS J17502484-0016151 system from the Sun?

The 2MASS J17502484-0016151 system is 30 light years or 9.2 parsecs from the Sun.

What galaxy is the 2MASS J17502484-0016151 star in?

The 2MASS J17502484-0016151 is in the Milky Way galaxy just like the Sun.

How many stars are in the 2MASS J17502484-0016151 system?

The 2MASS J17502484-0016151 is a single star, there are no other known stars in the system.

What type of star is the 2MASS J17502484-0016151?

The star 2MASS J17502484-0016151 is a Brown dwarf star.

What temperature is star 2MASS J17502484-0016151?

The star 2MASS J17502484-0016151 has an effective temperature of 1800 K. Find out more about the temperature of stars in Stellar guide
Class of stars Brown dwarf
Brown dwarfs are not really stars, because there is no thermonuclear fusion in their core. These objects are smaller and cooler than stars, but too massive to be considered planets.
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stellar brief logoStellar Brief

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27. 10. 2026
stellar brief logo
A giant planet candidate near Boyajian’s star may look oversized because a broad ring system surrounds it, not because the planet itself is unusually large. New atmospheric models also show why methane and carbon monoxide can vary across hot gas giants, exposing major limits in simpler predictions.
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